Poor Weather Queue Summary : Semester 2018B GN |
The queues shown in the tables below summarise the programs that constitute the "Poor Weather Queue" on GN. The Poor Weather Queue is a pilot program introduced in 2006B to fill telescope time under very poor, but usable, conditions. These programs are distinct from other queue programs in three important ways: 1) time spent on poor weather programs will not be charged to the PIs or the partner countries; 2) poor weather programs can exist in queue only, and must meet the observing condition constraints shown below; and 3) poor weather programs are lower priority than the "regular" queue (bands 1 to 3) and have no explicit or implicit guarantee of being observed. They will be executed only when nothing in the regular queue is observable.
In all other respects — NGO and Gemini contact scientist support, Phase II definitions, Gemini Science Archive data distribution — programs in the Poor Weather Queue are similar to all other Gemini queue programs. In the Observing Tool, poor weather queue programs are designated as Band 4, to distinguish them from the rest of the queue.
Observing condition constraints for poor weather programs must meet one of the following:
This report is generated daily (see the bottom of the page for the current timestamp). The pages linked via Completion Status are updated approximately every 4 hours. Note that the completion fraction may change as the time accounting is adjusted during the quality assessment process.
The assigned support staff (Gemini Contact Scientists and National Office staff) for each Gemini North ODB and Gemini South ODB program are listed in the interactive 'snapshots' of the Observing Database (ODB).
GN Poor Weather Queue | ||||||
Ref # | PI | Partner | Title | Instrument | Hours allocated |
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GN-2018B-Q-401 | Investigator | GS | Second spectrum for Kojima event | GMOS | 1.00 | |
Execution Status: | Dates Taken: 20180830 20181218 20181231 |
Completion Status:
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GN-2018B-Q-402 | Salinas | GS | Weighing the nearest elliptical galaxy | GMOS | 31.90 | |
Execution Status: | Dates Taken: |
Completion Status:
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GN-2018B-Q-403 | Placco | GS | Finding the brightest low-metallicity stars between the clouds | GMOS / GMOS-S | 20.00 | |
Execution Status: | Dates Taken: 20181107 20181214 20181218 20190118 20190119 20190302 20190306 20190310 20190325 20190428 20190520 20190604 20190605 |
Completion Status:
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GN-2018B-Q-404 | Chene | GS | Characterizing line profile variations in Wolf-Rayet stars | GMOS | 12.70 | |
Execution Status: | Dates Taken: 20180914 20180917 20181016 20181017 20181124 |
Completion Status:
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GN-2018B-Q-405 | Weidmann | GS | Central Stars of Planetary Nebulae: Survey for Spectral Classification | GMOS | 11.50 | |
Execution Status: complete | Dates Taken: 20181005 20181010 20181015 20181016 20181101 20181111 20181115 20181116 20190118 |
Completion Status:
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GN-2018B-Q-406 | Xu | GS | The Gaia View of Dust Disks around White Dwarfs | Flamingos2 / NIRI | 20.10 | |
Execution Status: | Dates Taken: 20181204 20181205 20181211 20181212 20181213 20181214 20190118 |
Completion Status:
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GN-2018B-Q-407 | Schimoia | BR | Monitoring of the broad Balmer double-peaked emission lines of NGC4203 and NGC4450 | GMOS | 42.00 | |
Execution Status: | Dates Taken: 20181107 20190530 20190602 |
Completion Status:
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GN-2018B-Q-408 | Molina Lera | GS | Early stellar population of seven open clusters in the second Galactic quadrant | GMOS | 20.00 | |
Execution Status: | Dates Taken: 20181204 20181205 20181211 20181214 20181215 20181216 20190107 |
Completion Status:
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GN-2018B-Q-409 | Arias | GS | Time evolution of EW Lac's circumstellar envelope | GNIRS | 0.70 | |
Execution Status: | Dates Taken: 20181218 |
Completion Status:
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GN-2018B-Q-410 | Arias | GS | CO emission from the Yellow Hypergiant Rho Cas | GNIRS | 2.10 | |
Execution Status: | Dates Taken: 20181220 |
Completion Status:
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Last updated on: 7 Jun 2021 17:21:48 GMT